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Statistical mechanics of geophysical turbulence: application to Jovian flows and Jupiter's great red spot

机译:地球物理湍流的统计力学:在木星流和木星大红点中的应用

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We propose a parameterization of 2D geophysical turbulence in the form of a relaxation equation similar to a generalized Fokker-Planck equation [P.H. Chavanis, Phys. Rev. E 68 (2003) 036108]. This equation conserves circulation and energy and increases a generalized entropy functional determined by a prior vorticity distribution fixed by small-scale forcing [R. Ellis, K. Haven, B. Turkington, Nonlinearity 15 (2002) 239]. We discuss applications of this formalism to jovian atmosphere and Jupiter's great red spot. We show that, in the limit of small Rossby radius where the interaction becomes short-range, our relaxation equation becomes similar to the Cahn-Hilliard equation describing phase ordering kinetics. This strengthens the analogy between the jet structure of the great red spot and a "domain wall". Our relaxation equation can also serve as a numerical algorithm to construct arbitrary nonlinearly dynamically stable stationary solutions of the 2D Euler equation. These solutions can represent jets and vortices that emerge in 2D turbulent flows as a result of violent relaxation. Due to incomplete relaxation, the statistical prediction may fail and the system can settle on a stationary solution of the 2D Euler equation which is not the most mixed state. In that case, it can be useful to construct more general nonlinearly dynamically stable stationary solutions of the 2D Euler equation in an attempt to reproduce observed phenomena. (C) 2004 Elsevier B.V. All rights reserved.
机译:我们提出了以类似于广义Fokker-Planck方程[P.H.]的弛豫方程的形式对2D地球物理湍流进行参数化。 Chavanis,物理学。 Rev E 68(2003)036108]。该方程式节省了循环和能量,并增加了由小规模强迫固定的先验涡度分布所确定的广义熵泛函[R。 Ellis,K.Haven,B.Turkington,Nonlinearity 15(2002)239]。我们讨论了这种形式主义在木星气氛和木星的大红点中的应用。我们证明,在相互作用变为短程的小Rossby半径范围内,我们的弛豫方程变得类似于描述相序动力学的Cahn-Hilliard方程。这加强了大红色斑点的射流结构与“畴壁”之间的类比。我们的松弛方程还可以用作数值算法来构造二维Euler方程的任意非线性动态稳定平稳解。这些解决方案可以代表由于剧烈松弛而在2D湍流中出现的喷流和涡流。由于不完全松弛,统计预测可能会失败,并且系统可能会以二维Euler方程的固定解(不是最混合的状态)为基础。在那种情况下,构造二维Euler方程的更一般的非线性动态稳定平稳解可能会很有用,以尝试重现观察到的现象。 (C)2004 Elsevier B.V.保留所有权利。

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